Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Redshift, Galaxy cluster, Weak gravitational lensing, and Galaxy.
Optical cluster cosmology with SDSS redMaPPer clusters and HSC-Y3 lensing measurements
X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton
Galaxy populations in the most distant SPT-SZ clusters
Weak-lensing analysis of SPT-selected galaxy clusters using Dark Energy Survey Science Verification data
Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at 1.4 ≲ z ≲ 1.7
Baryon content in a sample of 91 galaxy clusters selected by the South Pole Telescope at 0.2 <z < 1.25
Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 <
DSpace@MIT (Massachusetts Institute of Technology) 2018cited by 66position: middle
Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to<i>z</i> = 1.3
Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev–Zel'dovich Survey
Galaxy Populations in Massive Galaxy Clusters to $z$ = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
STAR-FORMING BRIGHTEST CLUSTER GALAXIES AT 0.25 < z < 1.25: A TRANSITIONING FUEL SUPPLY
DSpace@MIT (Massachusetts Institute of Technology) 2017cited by 46position: middle
Optical–SZE scaling relations for DES optically selected clusters within the SPT-SZ Survey
COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY
Detection of the kinematic Sunyaev–Zel'dovich effect with DES Year 1 and SPT
SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY
Detection of enhancement in number densities of background galaxies due to magnification by massive galaxy clusters
GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY
MASS CALIBRATION AND COSMOLOGICAL ANALYSIS OF THE SPT-SZ GALAXY CLUSTER SAMPLE USING VELOCITY DISPERSION σ<sub><i>v</i></sub>AND X-RAY<i>Y</i><sub>X</sub>MEASUREMENTS
Constraints on the richness–mass relation and the optical-SZE positional offset distribution for SZE-selected clusters
A MEASUREMENT OF GRAVITATIONAL LENSING OF THE COSMIC MICROWAVE BACKGROUND BY GALAXY CLUSTERS USING DATA FROM THE SOUTH POLE TELESCOPE
Baryon content of massive galaxy clusters at 0.57 < <i>z</i> < 1.33
Constraints on the CMB temperature evolution using multiband measurements of the Sunyaev–Zel'dovich effect with the South Pole Telescope